activity
20142026
most citedLITTLE THINGS in 3D: robust determination of the circular velocity of dwarf irregular galaxies

120 citations · 760 across the 26 of their papers we have counts for

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Showing 2023Show all

6 papers · 1 filter

astro-ph.GA2023★ 1 cited

A Galactic Eclipse: The Small Magellanic Cloud is Forming Stars in Two, Superimposed Systems

Claire E. Murray, Sten Hasselquist, Joshua E. G. Peek +22

The structure and dynamics of the star-forming disk of the Small Magellanic Cloud (SMC) have long confounded us. The SMC is widely used as a prototype for galactic physics at low m…

astro-ph.GA2023★ 6 cited

The JWST Galactic Center Survey -- A White Paper

Rainer Schoedel, Steve Longmore, Jonny Henshaw +111

The inner hundred parsecs of the Milky Way hosts the nearest supermassive black hole, largest reservoir of dense gas, greatest stellar density, hundreds of massive main and post ma…

astro-ph.GA2023★ 21 cited

MOKA3D: An innovative approach to 3D gas kinematic modelling. I. Application to AGN ionized outflows

C. Marconcini, A. Marconi, G. Cresci +15

Studying the feedback process of Active Galactic Nuclei (AGN) requires characterising multiple kinematical components, such as rotating gas and stellar disks, outflows, inflows, an…

astro-ph.GA2023★ 18 cited

Direct observations of the atomic-molecular phase transition in the Milky Way's nuclear wind

Karlie A. Noon, Mark R. Krumholz, Enrico M. Di Teodoro +3

Hundreds of high-velocity atomic gas clouds exist above and below the Galactic Centre, with some containing a molecular component. However, the origin of these clouds in the Milky…

astro-ph.GA2023★ 43 cited

Cold gas disks in main-sequence galaxies at cosmic noon: Low turbulence, flat rotation curves, and disk-halo degeneracy

Federico Lelli, Zhi-Yu Zhang, Thomas G. Bisbas +6

We study the dynamics of cold molecular gas in two main-sequence galaxies at cosmic noon (zC-488879 at and zC-400569 at ) using new high-resolution ALMA…

astro-ph.HE2023★ 19 cited

Study of the excess Fe XXV line emission in the central degrees of the Galactic centre using XMM-Newton data

K. Anastasopoulou, G. Ponti, M. C. Sormani +14

The diffuse Fe XXV (6.7 keV) line emission observed in the Galactic ridge is widely accepted to be produced by a superposition of a large number of unresolved X-ray point sources.…